© CSIRO 2002AbstractAn examination is made of the relationship between the observed energy spectrum of cosmic rays and the averaged spectrum of the cosmic rays at their sources. These spectra differ greatly, due to propagation effects. A form of the source spectrum is deduced which is a rather featureless power law over the full range of observations from 1010 eV to 1020 eV. We suggest that this lack of features is indicative of a common source for all cosmic rays over the full energy range, as opposed to lower energy Galactic and higher energy intergalactic components such as is often suggested.</jats:p
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
AbstractInvestigations of the energy spectrum as well as the mass composition of cosmic rays in the ...
One of several working groups established for this workshop was charged with examining results and m...
Abstract: It is generally believed that the cosmic rays below the ankle of the energy spectrum are o...
The cosmic ray energy spectrum is calculated assuming that cosmic rays are generated by astro-physic...
The energy spectrum of cosmic rays with primary energies between 1014 eV and 1016 eV has been studie...
This plot shows a compilation of the cosmic-ray energy spectrum measured by several experiments (not...
A spectrum of cosmic rays within energy range 1015 − 3 × 1017 eV was derived from the data of the sm...
Spectrum of cosmic rays follows a broken power law over twelve orders of magnitude. Since ubiquitous...
We begin with a brief introduction of the cosmic ray energy spectrum and its main features. At energ...
Contains fulltext : 92447.pdf (publisher's version ) (Open Access
The energy spectrum of cosmic rays between 10(16) eV and 10(18) eV, derived from measurements of the...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
The Galactic cosmic ray spectrum is a remarkably straight power law. Our current understanding is th...
The works on this subject usually refer to the so-called. averaged spectra. The authors try to bypas...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
AbstractInvestigations of the energy spectrum as well as the mass composition of cosmic rays in the ...
One of several working groups established for this workshop was charged with examining results and m...
Abstract: It is generally believed that the cosmic rays below the ankle of the energy spectrum are o...
The cosmic ray energy spectrum is calculated assuming that cosmic rays are generated by astro-physic...
The energy spectrum of cosmic rays with primary energies between 1014 eV and 1016 eV has been studie...
This plot shows a compilation of the cosmic-ray energy spectrum measured by several experiments (not...
A spectrum of cosmic rays within energy range 1015 − 3 × 1017 eV was derived from the data of the sm...
Spectrum of cosmic rays follows a broken power law over twelve orders of magnitude. Since ubiquitous...
We begin with a brief introduction of the cosmic ray energy spectrum and its main features. At energ...
Contains fulltext : 92447.pdf (publisher's version ) (Open Access
The energy spectrum of cosmic rays between 10(16) eV and 10(18) eV, derived from measurements of the...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
The Galactic cosmic ray spectrum is a remarkably straight power law. Our current understanding is th...
The works on this subject usually refer to the so-called. averaged spectra. The authors try to bypas...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
AbstractInvestigations of the energy spectrum as well as the mass composition of cosmic rays in the ...
One of several working groups established for this workshop was charged with examining results and m...